A 104-kDa diacylglycerol kinase containing ankyrin-like repeats localizes in the cell nucleus.

The cDNA corresponding to a fourth species of diacylglycerol (DG) kinase (EC 2.7.1.107) was isolated from cDNA libraries of rat retina and brain. This cDNA encoded a 929-aa, 104-kDa polypeptide termed DGK-IV. DGK-IV was different from previously identified mammalian DG kinase species, DGK-I, DGK-II, and DGK-III, in that it contained no EF-hand motifs but did contain four ankyrin-like repeats at the carboxyl terminus. These structural features of DGK-IV closely resemble the recently cloned, eye-specific DG kinase of Drosophila that is encoded by the retinal degeneration A (rdgA) gene. However, DGK-IV was expressed primarily in the thymus and brain with relatively low expression in the eye and intestine. Furthermore, the primary structure of the DGK-IV included a nuclear targeting motif, and immunocytochemical analysis revealed DGK-IV to localize in the nucleus of COS-7 cells transfected with the epitope-tagged cDNA, suggesting an involvement of DGK-IV in intranuclear processes.

Pathways to quiescence: SHARDS view on the star formation histories of massive quiescent galaxies at 1.0 < z < 1.5

We present star formation histories (SFHs) for a sample of 104 massive (stellar mass M > 10^10 M_⊙) quiescent galaxies (MQGs) at z = 1.0–1.5 from the analysis of spectrophotometric data from the Survey for High-z Absorption Red and Dead Sources (SHARDS) and HST/WFC3 G102 and G141 surveys of the GOODS-North field, jointly with broad-band observations from ultraviolet (UV) to far-infrared (far-IR). The sample is constructed on the basis of rest-frame UVJ colours and specific star formation rates (sSFRs = SFR/Mass). The spectral energy distributions (SEDs) of each galaxy are compared to models assuming a delayed exponentially declining SFH. A Monte Carlo algorithm characterizes the degeneracies, which we are able to break taking advantage of the SHARDS data resolution, by measuring indices such as MgUV and D4000. The population of MQGs shows a duality in their properties. The sample is dominated (85 per cent) by galaxies with young mass-weighted ages, t_M t_M < 2 Gyr, short star formation time-scales, 〈τ〉 ∼ 60–200 Myr, and masses log(M/M_⊙) ∼ 10.5. There is an older population (15 per cent) with t_M t_M = 2–4 Gyr, longer star formation time-scales, 〈τ〉∼ 400 Myr, and larger masses, log(M/M_⊙) ∼ 10.7. The SFHs of our MQGs are consistent with the slope and the location of the main sequence of star-forming galaxies at z > 1.0, when our galaxies were 0.5–1.0 Gyr old. According to these SFHs, all the MQGs experienced a luminous infrared galaxy phase that lasts for ∼500 Myr, and half of them an ultraluminous infrared galaxy phase for ∼100 Myr. We find that the MQG population is almost assembled at z ∼ 1, and continues evolving passively with few additions to the population.

La Direttiva 2008/104/CE relativa al lavoro tramite agenzia interinale: aspetti problematici e modelli di implementazione = Directive 2008/104/EC relating to temporary agency work: problematic aspects and implementation models. WP C.S.D.L.E. “Massimo D’Antona”.INT – 101/2013

The problematic gestation of the Directive on temporary agency work shows the presence of several criticalities that there are also in the national transposition in relation to the principle of equal treatment and to the mechanisms for preventing abuse during successive assignments. From a first analysis it can be said that in some EU Member States only the derogations have been implemented and not the general principle of equal treatment. At the same time, the obligation of the Member States, contained in the Directive on temporary agency work, to establish mechanisms for preventing abuse during successive assignments is crucial, especially in the light of the recent case law of the EU Court of Justice in which the Court does not apply to the temporary agency workers the protective rules of the Directive on fixed-term contracts (see C-290/12 , Della Rocca).